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Introduction to Physics

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Title: Introduction to Physics


1
Chapter 1 Introduction to Physics
Image of Sun from STEREO, from NASA.
2
1-1 Physics and the Laws of Nature
  • Physics the study of the fundamental laws of
    nature
  • these laws can be expressed as mathematical
    equations
  • much complexity can arise from relatively simple
    laws

3
1-2 Units of Length, Mass, and Time
SI units of length (L), mass (M), time
(T) Length the meter (or metre) Was one
ten-millionth of the distance from the North Pole
to the equator Now the distance traveled by
light in a vacuum in 1/299,792,458 of a second
(set by The International System of
Units) http//www.bipm.org/en/si/ Mass the
kilogram One kilogram is the mass of a particular
platinum-iridium cylinder kept at the
International Bureau of Weights and Standards,
Sèvres, France. Time the second One second is
the time for radiation from a cesium-133 atom to
complete 9,192,631,770 oscillation cycles.
4
1-2 Units of Length
http//en.wikipedia.org/wiki/Orders_of_magnitude_
28length29
5
1-2 Units of Length
There is Plenty of Room at the Bottom Feynmann
http//en.wikipedia.org/wiki/Orders_of_magnitude_
28length29
6
1-2 Units of Mass
7
1-2 Units of Time
8
1-2 Units of Length, Mass, and Time
9
1-3 Dimensional Analysis
  • Any valid physical formula must be dimensionally
    consistent each side must have the same
    dimensions

From the table Distance velocity
time Velocity acceleration time Energy mass
(velocity)2
10
1-4 Significant Figures
  • accuracy of measurements is limited
  • significant figures the number of digits in a
    quantity that are known with certainty
  • number of significant figures after
    multiplication or division is the number of
    significant figures in the least-known quantity

11
1-4 Significant Figures
  • Scientific Notation
  • Leading or trailing zeroes can make it hard to
    determine number of significant figures 2500,
    0.000036
  • Each of these has two significant figures
  • Scientific notation writes these as a number
    from 1-10 multiplied by a power of 10, making the
    number of significant figures much clearer
  • 2500 2.5 103
  • If we write 2.50x103, it has three significant
    figures
  • 0.000036 3.6 x 10-5

12
1-4 Significant Figures
Round-off error The last digit in a calculated
number may change depending on how it is
calculated, due to rounding off of insignificant
digits, might lead to big errors. Example 12.46
6 tax 13.2076, rounds to 13.21 1.76 6
tax 1.8656, rounds to 1.87 Sum 13.21 1.87
15.08 12.46 1.76 14.22 14.22 6 tax
15.07
13
1-5 Converting Units
WE WILL NOT DEAL WITH IMPERIAL SYSTEM. YOU DO NOT
NEED TO KNOW CONVERSION FOR THAT.
1 hour 60 minutes 3600 seconds 1 km 1000
m 1 cm 0.01 m 1 mm 0.001 m
14
1-6 Order-of-Magnitude Calculations
  • Why are estimates useful?
  • as a check for a detailed calculation if your
    answer is very different from your estimate,
    youve probably made an error
  • to estimate numbers where a precise calculation
    cannot be done

15
1-7 Scalars and Vectors
Scalar a numerical value. May be positive or
negative. Examples temperature, speed, height,
your age or weight. Vector a scalar with
direction. Examples displacement (e.g., 10 feet
north), force, magnetic field
16
1-8 Problem Solving in Physics
  • No recipe or plug-and-chug works all the time,
    but here are some guidelines
  • A - Understand The Question
  • Read the problem carefully
  • Sketch the system
  • Visualize the physical process
  • Strategize
  • B - Solve The Question
  • Identify appropriate equations
  • Solve the equations
  • Check your answer
  • Explore limits and special cases

17
Bottom Line of Chapter 1
  • Physics is based on a small number of laws and
    principles
  • Units of length are meters of mass, kilograms
    and of time, seconds in this course.
  • Equations must have same dimensions on each
    side.
  • The result of a calculation should have only as
    many significant figures as the least accurate
    measurement used in it

18
Bottom Line of Chapter 1
  • Convert your units to a set of useful ones before
    doing anything else
  • Order-of-magnitude calculations are designed to
    be accurate within a power of 10
  • Scalars are just numbers vectors are scalars
    with direction.
  • Problem solving understanding the problem is
    the main step, read, sketch etc., then see which
    formulas would be useful.
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